Gema Araujo caught this wonderful solar prominence on September 2, 2007 at 08:56 UT. More of Gema's images can be seen at www.astrosurf.com/obsolar/.
Canadian solar observers Ralph Chou and John Ginder recorded four hours of solar prominence activity on September 23, 2007. They captured about 30GB of data, stacked the 40 best frames and produced a wonderful 5 second movie clip that is posted on YouTube. http://www.youtube.com/watch?v=PNabV7qHtkE
The timestamp in their clip is EDT (Eastern Daylight Time) You'll notice details come and go which they didn't see live on their screen until they produced the movie.This is an amazing effort with a 3 inch telescope, a Coronado filter, 4X Barlow and Lumenera camera. Hopefully other observers will give it a try.
Remember to send me any solar drawings, SID flares or photos for me to include here.
Sudden Ionospheric Disturbance Report
Michael Hill, SID Analyst
114 Prospect St
Marlborough, MA 01752 USA
noatak@aol.com
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Sudden Ionospheric Disturbances (SID)
Recorded During September 2007
(Analysis performed by Michael Hill, SID Analyst)
| Importance rating: Duration | -1: <19 | 1: 19-25 | 1+: 26-32 | 2: 33-45 | 2+: 46-85 | 3: 86-125 | 3+: >125 |
| Observer |
Code |
Station(s) monitored |
| P King |
A80 |
NAA |
| M Hill |
A87 |
NAA |
| R Battaiola |
A96 |
HWU |
| J Wallace |
A97 |
NAA |
| M King |
A99 |
HWU |
| F Steyn |
A102 |
NAA NWC |
| L Observatory |
A107 |
DHO |
| P Mortfield |
A108 |
NAA |
| L Loudet |
A118 |
DHO |
| J Godet |
A119 |
GBZ GQD ICV |
The events listed above meet at least one of the following criteria
- Event reported by two or more observers within +/- 5 minutes
- Event matched to GOES-8 XRA event to within +/- 15 minutes and event time < 1000 UT
- Reported by observer with a high quality rating > 8 (scale 1-10)
September was a very slow month for SID activity. In fact there was no activity. As you can see there is no bar graph to the upper right as there usually is because there were 0 correlated SID events submitted by our observers. Even the GOES-12 Data shows a dearth of X-Ray flares. There were only 16 this past month and all but three were B class events. The others still only C Class at that.
All reports submitted to me were that of NO SID's detected. All except mine. As is depicted in the graph on the previous page I did register something towards the end of the day. It sure looks like a SID event but there were no X-Ray flares recorded that day or other observations by observers to correlate with. This is one of those rare cases where an event that seems important goes unreported. It may seem like the wrong way to go but it is in fact consistent with the data set that goes back many years now. To report it would be to change the criteria that we use and therefore skew the data. It couldn't have been a SID. In fact I have two systems running and the other did not record it. This highlights the fact that not every event you see is in fact a SID. There are other factors at work and on occasion the effect of these factors will appear as a SID signature. This is why we correlate with other observers and why it is good to have many observers to cross correlate with. So keep on monitoring. Your sumbissions are always important even when the times are slow. And slow they are at these days.
Solar Flare Summary Based on GOES-12 Data
Sunspot Data
American Relative Sunspot Numbers(Ra) for September 2007 [boldface = maximum, minimum]
| Day |
N |
Raw
Mean |
Ra |
| 1 |
44 |
22 |
16 |
| 2 |
40 |
14 |
11 |
| 3 |
44 |
11 |
8 |
| 4 |
33 |
10 |
7 |
| 5 |
41 |
10 |
7 |
| 6 |
33 |
3 |
2 |
| 7 |
36 |
0 |
0 |
| 8 |
40 |
0 |
0 |
| 9 |
30 |
0 |
0 |
| 10 |
32 |
0 |
0 |
| 11 |
39 |
0 |
0 |
| 12 |
32 |
0 |
0 |
| 13 |
33 |
0 |
0 |
| 14 |
35 |
1 |
0 |
| 15 |
43 |
0 |
0 |
| 16 |
41 |
0 |
0 |
| 17 |
34 |
0 |
0 |
| 18 |
32 |
0 |
0 |
| 19 |
30 |
0 |
0 |
| 20 |
34 |
0 |
0 |
| 21 |
34 |
0 |
0 |
| 22 |
30 |
0 |
0 |
| 23 |
39 |
0 |
0 |
| 24 |
37 |
1 |
0 |
| 25 |
38 |
0 |
0 |
| 26 |
36 |
0 |
0 |
| 27 |
30 |
3 |
2 |
| 28 |
34 |
14 |
11 |
| 29 |
24 |
15 |
10 |
| 30 |
27 |
14 |
11 |
Means |
35.2 |
3.9 |
2.8 |
Total No. of Observers: 58
Total No. of Observations: 1055
|
September 2007 Sunspot Observers
| AAP |
A. Abbott |
19 |
| AJV |
J. Alonso |
17 |
| ANGR |
R. Ang |
30 |
| BARH |
H. Barnes |
11 |
| BATR |
R. Battaiola |
10 |
| BEB |
R. Berg |
10 |
| BEDJ |
J. Bedient |
15 |
| BMF |
M. Boschat |
21 |
| BRAB |
B. Branchett |
27 |
| BRAD |
D. Branchett |
17 |
| BRAR |
R. Branch |
28 |
| BROB |
R. Brown |
29 |
| BVC |
A. Buck |
30 |
| CHAG |
G. Morales |
27 |
| CKB |
B. Cudnik |
28 |
| CLZ |
L. Corp |
19 |
| CNT |
D. Chantiles |
7 |
| COMT |
T. Compton |
19 |
| CVJ |
J. Carvajal |
24 |
| DEJV |
J. van Delft |
18 |
| DGP |
G. Dyck |
13 |
| DUBF |
F. Dubois |
27 |
| FERJ |
J. Fernandez |
15 |
| FLET |
T. Fleming |
26 |
| GFT |
F. Gobet |
12 |
| GOEM |
M. Goetz |
1 |
| HALB |
B. Halls |
10 |
| HAYK |
K. Hay |
15 |
| HMQ |
M. Harris |
18 |
| KAPJ |
J. Kaplan |
25 |
| KNJS |
J. & S. Knight |
15 |
| KROL |
L. Krozel |
5 |
| KUZM |
M. Kuzmin |
4 |
| LERM |
M. Lerman |
12 |
| MARJ |
J. Maranon |
23 |
| MCE |
E. Mochizuki |
21 |
| MCHL |
L. McHenry |
3 |
| MEU |
E. Mason |
4 |
| MILJ |
J. Miller |
18 |
| MMI |
M. Moeller |
23 |
| OATS |
S. Oatney |
17 |
| OBSO |
IPS Observatory |
18 |
| RICE |
E. C. Richardson |
15 |
| RITA |
A. Ritchie |
18 |
| SCGL |
G. Schott |
29 |
| SIMC |
C. Simpson |
12 |
| STEM |
G. Stemmler |
17 |
| STQ |
N. Stoikidis |
24 |
| SUZM |
M. Suzuki |
24 |
| SZUM |
M. Szulc |
24 |
| TESD |
D. Teske |
24 |
| TJV |
J. Temprano |
23 |
| URBP |
P. Urbanski |
22 |
| VARG |
A. Vargas |
24 |
| VIDD |
D. Vidican |
18 |
| WILW |
W. Wilson |
21 |
| WRP |
R. Wheeler |
4 |
| YESH |
H. Yesilyaprak |
25 |
|
|
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Reporting addresses:
Sunspot Reports
Email: solar@aavso.org
Postal Mail: AAVSO,
49 Bay State Rd. Cambridge, MA, 02138
Fax: 617-354-0665
SID Flare Reports
Email: noatak@aol.com
Postal Mail: Mike Hill,
114 Prospect St., Marlboro, MA, 01752
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Smoothed Mean Sunspot Numbers (Rsm) from January 2000 to March 2007 (Waldmeier method). |
 |
10 cm Solar Flux and American Relative Sunspot Numbers (Ra) for September 2007
(10cm Source: http://www.drao.nrc.ca/icarus) |
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